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Record W3201222696 · doi:10.1093/mnras/stab2679

Observations of compact sources in galaxy clusters using MUSTANG2

2021· article· en· W3201222696 on OpenAlexafffund
Simon Dicker, E. S. Battistelli, Tanay Bhandarkar, Mark J. Devlin, Shannon M. Duff, G. C. Hilton, Matt Hilton, Adam D. Hincks, Johannes Hubmayr, K. M. Huffenberger, John P. Hughes, Luca Di Mascolo, Brian Mason, John A. B. Mates, J. J. McMahon, Tony Mroczkowski, Sigurd Næss, John Orlowski-Scherer, Bruce Partridge, Federico Radiconi, C. Romero, Craig L. Sarazin, Neelima Sehgal, Jonathan Sievers, Cristobál Sifón, Joel N. Ullom, Leila R. Vale, Michael Vissers, Zhilei Xu

Bibliographic record

VenueArTS Archivio della ricerca di Trieste (University of Trieste https://www.units.it/) · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsMcGill UniversityUniversity of Toronto
FundersNational Institute of Standards and TechnologyAgencia Nacional de Investigación y DesarrolloUniversity of TorontoInyuvesi Yakwazulu-NataliNational Energy Research Scientific Computing CenterNational Aeronautics and Space AdministrationUniversity of PennsylvaniaCanada Foundation for InnovationNational Science FoundationCompute CanadaComisión Nacional de Investigación Científica y TecnológicaAssociated UniversitiesPrinceton UniversityGovernment of Ontario
KeywordsPhysicsAstrophysicsGalaxy clusterCluster (spacecraft)Flux (metallurgy)GalaxyCosmologyTelescopeAmplitudeSpectral indexAngular resolution (graph drawing)PopulationSource countsAstronomyRedshiftSpectral lineOptics

Abstract

fetched live from OpenAlex

Compact sources can cause scatter in the scaling relationships between the amplitude of the thermal Sunyaev-Zel'dovich Effect (tSZE) in galaxy clusters and cluster mass. Estimates of the importance of this scatter vary - largely due to limited data on sources in clusters at the frequencies at which tSZE cluster surveys operate. In this paper, we present 90 GHz compact source measurements from a sample of 30 clusters observed using the MUSTANG2 instrument on the Green Bank Telescope. We present simulations of how a source's flux density, spectral index, and angular separation from the cluster's centre affect the measured tSZE in clusters detected by the Atacama Cosmology Telescope (ACT). By comparing the MUSTANG2 measurements with these simulations we calibrate an empirical relationship between 1.4 GHz flux densities from radio surveys and source contamination in ACT tSZE measurements. We find 3 per cent of the ACT clusters have more than a 20 per cent decrease in Compton-y but another 3 per cent have a 10 per cent increase in the Compton-y due to the matched filters used to find clusters. As sources affect the measured tSZE signal and hence the likelihood that a cluster will be detected, testing the level of source contamination in the tSZE signal using a tSZE-selected catalogue is inherently biased. We confirm this by comparing the ACT tSZE catalogue with optically and X-ray-selected cluster catalogues. There is a strong case for a large, high-resolution survey of clusters to better characterize their source population.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.045
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.001
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0010.002
Science and technology studies0.0010.001
Scholarly communication0.0000.001
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.045
GPT teacher head0.227
Teacher spread0.182 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations11
Published2021
Admission routes2
Has abstractyes

Explore more

Same venueArTS Archivio della ricerca di Trieste (University of Trieste https://www.units.it/)Same topicGalaxies: Formation, Evolution, PhenomenaFrench-language works237,207